Some optical properties of rotating wormhole in Bopp-Podolsky electrodynamics
arXiv:2411.15782 · doi:10.1088/1475-7516/2025/04/065
Abstract
In this work, we consider a static wormhole in Bopp-Podolsky electrodynamics and convert it into its rotating counterpart by reducing it into Morris-Thorne form. We further study the null geodesics and effective potential along with the shadows for inner and outer unstable orbits for specific choices of parameters. It is found that for some cases smooth shadow curves are formed and for a few cases, the shadows formed are cuspy. All parameters have a significant impact on the shadows except for the parameter when either or are kept small. We also analyze the gravitational lensing in the strong regime, considering that the observer and the source are on opposite sides of the throat. For this situation, we explore in detail the behavior of the deflection angle, Einstein rings and lensing observables.
References in corpus (16)
- Relativistic images of Schwarzschild black hole lensing
- Generating rotating regular black hole solutions without complexification
- Strong deflection limit analysis and gravitational lensing of an Ellis wormhole
- Deflection angle in the strong deflection limit in a general asymptotically flat, static, spherically symmetric spacetime
- A comparison of approximate gravitational lens equations and a proposal for an improved new one
- Light's Bending Angle due to Black Holes: From the Photon Sphere to Infinity
- Testing wormhole solutions in extended gravity through the Poynting-Robertson effect
- General relativistic Poynting-Robertson effect to diagnose wormholes existence: static and spherically symmetric case
- Astrophysical Wormholes
- Classical and quantum stability of higher-derivative dynamics
- Spin, torsion and violation of null energy condition in traversable wormholes
- Geometry of Spinning Ellis Wormholes
- Exact rotating wormholes via Ehlers transformations
- Higher order derivative operators as quantum corrections
- Viable wormhole solution in Bopp-Podolsky electrodynamics
- Coulomb Law in the Non-Uniform Euler-Heisenberg Theory